Zobrazeno 1 - 10
of 270
pro vyhledávání: '"Ilie, Cosmin A."'
Autor:
Casey, Richard, Ilie, Cosmin
All of the significant evidence for dark matter observed thus far has been through its gravitational interactions. After 40 years of direct detection experiments, the parameter space for Weakly Interacting Massive Particles (WIMPs) as dark matter can
Externí odkaz:
http://arxiv.org/abs/2407.05752
Autor:
Ilie, Cosmin
Any astrophysical object can, in principle, serve as a probe of the interaction between Dark Matter and regular, baryonic matter. This method is based on the potential observable consequences annihilations of captured Dark Matter has on the surface t
Externí odkaz:
http://arxiv.org/abs/2402.07713
In this work we demonstrate that Dark Matter (DM) evaporation severely hinders the effectiveness of exoplanets and Brown Dwarfs as sub-GeV DM probes. Moreover, we find useful analytic closed form approximations for DM capture rates for arbitrary astr
Externí odkaz:
http://arxiv.org/abs/2312.13979
The James Webb Space Telescope (JWST) has recently uncovered a new record-breaking quasar, UHZ1, at a redshift of $z\sim10$. This discovery continues JWST's trend of confronting the expectations from the standard $\Lambda$CDM model of cosmology with
Externí odkaz:
http://arxiv.org/abs/2312.13837
Publikováno v:
ApJ 965 (2024) 121
The first bright objects to form in the Universe at redshift $z \sim 10-20$ might have been Dark Stars, made primarily of hydrogen and helium but powered by dark matter. In this study, we investigate the detectability of Supermassive Dark Stars (SMDS
Externí odkaz:
http://arxiv.org/abs/2306.11606
The first generation of stars in the Universe is yet to be observed. There are two leading theories for those objects that mark the beginning of the cosmic dawn: hydrogen burning Population~III stars and Dark Stars, made of hydrogen and helium but po
Externí odkaz:
http://arxiv.org/abs/2304.01173
Autor:
Ilie, Cosmin, Paulin, Jillian
Compact astrophysical objects have been considered in the literature as dark matter (DM) probes, via the observational effects of annihilating captured DM. In this respect, Population III (Pop III) stars are particularly interesting candidates, since
Externí odkaz:
http://arxiv.org/abs/2107.00675
Autor:
Ilie, Cosmin, Levy, Caleb
Publikováno v:
Phys. Rev. D 104, 083033 (2021)
In recent years, the usefulness of astrophysical objects as Dark Matter (DM) probes has become more and more evident, especially in view of null results from direct detection and particle production experiments. The potentially observable signatures
Externí odkaz:
http://arxiv.org/abs/2105.09765
Autor:
Ilie-Cosmin Cântar, Ersilia Alexa, Daniela Sabina Poșta, Vlad Emil Crişan, Nicolae Cadar, Adina Berbecea, Sándor Rózsa, Tincuța-Marta Gocan, Orsolya Borsai
Publikováno v:
Applied Sciences, Vol 14, Iss 12, p 5221 (2024)
The present article emphasizes the influence of forest vegetation on improving the content of toxic elements from soil, increasing the content of micro and macro elements as well as correlating these variations with characteristics of forest vegetati
Externí odkaz:
https://doaj.org/article/a239ddc40a924e959487f1498c305b9e
We show that the mere observation of the first stars (Pop III stars) in the universe can be used to place tight constraints on the strength of the interaction between dark matter and regular, baryonic matter. We apply this technique to a candidate Po
Externí odkaz:
http://arxiv.org/abs/2009.11478